Articles | Volume 18, issue 13
https://doi.org/10.5194/gmd-18-4215-2025
https://doi.org/10.5194/gmd-18-4215-2025
Model description paper
 | 
15 Jul 2025
Model description paper |  | 15 Jul 2025

A time-dependent three-dimensional dayside magnetopause model based on quasi-elastodynamic theory

Yaxin Gu, Yi Wang, Fengsi Wei, Xueshang Feng, Andrey Samsonov, Xiaojian Song, Boyi Wang, Pingbing Zuo, Chaowei Jiang, Yalan Chen, Xiaojun Xu, and Zilu Zhou

Related authors

Deep temporal convolutional networks for F10.7 radiation flux short-term forecasting
Luyao Wang, Hua Zhang, Xiaoxin Zhang, Guangshuai Peng, Zheng Li, and Xiaojun Xu
Ann. Geophys., 42, 91–101, https://doi.org/10.5194/angeo-42-91-2024,https://doi.org/10.5194/angeo-42-91-2024, 2024
Short summary
Latitudinal Dependence of the Geomagnetic and Solar Activity Effect on Sporadic-E layer
Qiong Tang, Chen Zhou, Huixin Liu, Yi Liu, Jiaqi Zhao, Zhibin Yu, Zhengyu Zhao, and Xueshang Feng
Atmos. Chem. Phys. Discuss., https://doi.org/10.5194/acp-2022-534,https://doi.org/10.5194/acp-2022-534, 2022
Preprint withdrawn
Short summary
Identification of slow magnetosonic wave trains and their evolution in 3-D compressible turbulence simulation
L. Zhang, L.-P. Yang, J.-S. He, C.-Y. Tu, L.-H. Wang, E. Marsch, and X.-S. Feng
Ann. Geophys., 33, 13–23, https://doi.org/10.5194/angeo-33-13-2015,https://doi.org/10.5194/angeo-33-13-2015, 2015

Related subject area

Earth and space science informatics
DustNet (v1): skilful neural network predictions of dust aerosols over the Saharan desert
Trish E. Nowak, Andy T. Augousti, Benno I. Simmons, and Stefan Siegert
Geosci. Model Dev., 18, 3509–3532, https://doi.org/10.5194/gmd-18-3509-2025,https://doi.org/10.5194/gmd-18-3509-2025, 2025
Short summary
RiverBedDynamics v1.0: a Landlab component for computing two-dimensional sediment transport and river bed evolution
Angel D. Monsalve, Samuel R. Anderson, Nicole M. Gasparini, and Elowyn M. Yager
Geosci. Model Dev., 18, 3427–3451, https://doi.org/10.5194/gmd-18-3427-2025,https://doi.org/10.5194/gmd-18-3427-2025, 2025
Short summary
A GPU parallelization of the neXtSIM-DG dynamical core (v0.3.1)
Robert Jendersie, Christian Lessig, and Thomas Richter
Geosci. Model Dev., 18, 3017–3040, https://doi.org/10.5194/gmd-18-3017-2025,https://doi.org/10.5194/gmd-18-3017-2025, 2025
Short summary
The Earth System Grid Federation (ESGF) Virtual Aggregation (CMIP6 v20240125)
Ezequiel Cimadevilla, Bryan N. Lawrence, and Antonio S. Cofiño
Geosci. Model Dev., 18, 2461–2478, https://doi.org/10.5194/gmd-18-2461-2025,https://doi.org/10.5194/gmd-18-2461-2025, 2025
Short summary
Can AI be enabled to perform dynamical downscaling? A latent diffusion model to mimic kilometer-scale COSMO5.0_CLM9 simulations
Elena Tomasi, Gabriele Franch, and Marco Cristoforetti
Geosci. Model Dev., 18, 2051–2078, https://doi.org/10.5194/gmd-18-2051-2025,https://doi.org/10.5194/gmd-18-2051-2025, 2025
Short summary

Cited articles

Agapitov, O., Glassmeier, K.-H., Plaschke, F., Auster, H.-U., Constantinescu, D., Angelopoulos, V., Magnes, W., Nakamura, R., Carlson, C. W., Frey, S., and McFadden, J. P.: Surface waves and field line resonances: A THEMIS case study, J. Geophys. Res.-Space, 114, A00C27, https://doi.org/10.1029/2008ja013553, 2009. 
Ala-Lahti, M., Pulkkinen, T. I., Pfau-Kempf, Y., Grandin, M., and Palmroth, M.: Energy Flux Through the Magnetopause During Flux Transfer Events in Hybrid-Vlasov 2D Simulations, Geophys. Res. Lett., 49, e2022GL100079, https://doi.org/10.1029/2022gl100079, 2022. 
Anderson, K. A., Binsack, J. H., and Fairfield, D. H.: Hydromagnetic disturbances of 3- to 15-minute period on magnetopause and their relation to bow shock spikes, J. Geophys. Res., 73, 2371–2386, https://doi.org/10.1029/JA073i007p02371, 1968. 
Angelopoulos, V.: The THEMIS mission, Space Sci. Rev., 141, 5–34, https://doi.org/10.1007/s11214-008-9336-1, 2008. 
Archer, M. O., Hartinger, M. D., and Horbury, T. S.: Magnetospheric “magic” frequencies as magnetopause surface eigenmodes, Nat. Commun., 40, 5003–5008, https://doi.org/10.1002/grl.50979, 2013. 
Download
Short summary
Understanding how solar wind interacts with Earth’s protective magnetic shield is a frontier issue in space physics, critical for predicting space weather risks. However, most existing magnetopause models cannot capture this time-dependent process, and numerical simulations demand significant computational resources. We have developed the first time-dependent 3D model capable of showing these shield changes. It is significantly more precise and performs nearly instant computations.
Share